Hα observations of Be stars
Astronomy and Astrophysics Division, Physical Research Laboratory, Navrangpura, Ahmedabad 380 009, India
Send offprint request to: D.P.K. Banerjee, e-mail: firstname.lastname@example.org
Accepted: 11 September 2000
We present here the Hα spectra of 44 Be stars taken at a resolution of 0.5 Å. From the spectra, different emission line parameters have been deduced. A study of the correlations between different pairs of these parameters has been made with a view to understanding the mechanisms of line formation and shaping in Be stars.
Key words: Be stars / spectroscopy / line profiles
© European Southern Observatory (ESO), 2000